NGC1068 LST1 analysis Cycle I DanielMorcuende
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Analysis of LST-1 NGC 1068 data from observation cycle I
General information
- Name of the source: NGC 1068
- Brief description of the source:
- Object type : Unknown, AGN, SNR, Pulsar, PWN, GRB, etc
- Redshift (z) :
- Other relevant information
- RA: XX XX XX.XX (hh mm ss), Dec: +/-YY YY YY.YY (dd mm ss)
- RA, Dec in deg (ICRS): XX.XX, YY.YY
- Analysis by Name (Institute - email)
- Daniel Morcuende
- José Manuel
Data-taking information
- Dates of data-taking:
- Date (time of observation h)
- ZD range (deg): Zenith Range
- AZ range (deg): Azimuth Range
- Runs:
- Date (time of observation h)
Monte Carlo information
- Link to MC files used:
- Particle types:
- ZD (deg): Zenith Range
- AZ (deg): Azimuth Range
DL1 data
Reprocessed using DL1a files produced by LSTOSA (lstchain v0.7.3) and dl1ab script (v0.7.5)
- original DL1a files
/fefs/aswg/data/real/DL1/20210808/v0.7.3/tailcut84/dl1_LST-1.Run0XXXX.XXXX.h5 /fefs/aswg/data/mc/DL1/20200629_prod5_trans_80/XXX/zenith_20deg/south_pointing/20210416_v0.7.3_prod5_trans_80_local_taicut_8_4/
- lstchain v0.7.5
- real data: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning
/fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/lstchain_standard_config.json
- MC: tailcut8-4 (with cleaning based on pedestal RMS), dynamic cleaning, PSF+NSB tuning
"image_modifier": { "increase_nsb": true, "extra_noise_in_dim_pixels": 0.74, "extra_bias_in_dim_pixels": 0.38, "transition_charge": 8, "extra_noise_in_bright_pixels": 0.052, "increase_psf": true, "smeared_light_fraction": 0.125 },
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/lstchain_dl1ab_tune_MC_to_BLLac_config.json
- Produced DL1b files
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/DL1_raw/data/ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/DL1_raw/Run0XXXX
Random forest
Please include your specific .json files used in producing your RFs and for which source analysis (source dependent or independent), and variables used in the RF.
DL2 data
- lstchain-v0.10
- source-indep
/fefs/aswg/workspace/seiya.nozaki/data/MC/v0.7.5/tailcut84_dynamic_bllac/srcindep/DL2/data/ /fefs/aswg/workspace/seiya.nozaki/data/BLLac/v0.7.3/tailcut84_dynamic_v075/srcindep/DL2/data/dl2_LST-1.Run0XXXX_merged.h5
DL3 data selection
Information about your DL3 data selection.
Example
- intensity > 50
- r: [0, 1 ]
- wl: [0.1, 1 ]
- leakage_intensity_width_2: [0, 0.2 ]
- source-indep
High-level analysis
- lstchain to generate source-dep IRF, DL3
- Science Tool: Gammapy 1.1
- point-like IRF, 1D analysis
Analysis Results
Please place higher-level analysis results (Spectra, SkyMaps, Lightcurves, etc) here.